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Super-luminous supernova (SLSN) are supernovae showing extreme properties intheir light-curves: high peak luminosities (more than 10 times brighter thanbright SN Ia), and long durations. Several mechanisms have been proposed forSLSN, such as pair instability SN of a massive progenitor, interaction of theejecta with a massive circumstellar shell, and the dual-shock quark nova (dsQN)model. The dual-shock quark nova model is unique in that it predicts a normalSN event will be seen about 10 days prior to the main SLSN event. The dsQNmodel is described here and shown that it is consistent with the light curve ofthe one currently known double-humped SLSN, 2006oz.

Double-humped Super-luminous Supernovae